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Explanation: Using the formula for minimum deviation in a prism: n = sin[(A + δm)/2] / sin(A/2), where A is the prism angle and δm is the angle of minimum deviation. Here, n = sin[(60° + 40°)/2] / sin(60°/2) ≈ 1.53.
Explanation: The angle of minimum deviation changes when the prism is immersed in water due to the change in relative refractive index. The formula for minimum deviation in a new medium is adjusted accordingly, resulting in an approximate angle of 30°.
Explanation: Using the lensmaker’s formula, 1/f = (n-1)(1/R1 - 1/R2). For a double-convex lens with equal radii, R1 = R2 = R. Solving for R, we get R = 2f(n-1) = 2 * 20 cm * (1.55 - 1) = 31 cm (approx).
Explanation: Since the beam converges at point P, which is 12 cm from the lens, and the focal length of the lens is 20 cm, the lens will bring the converging rays to a focus 12 cm on the other side of the lens.
Explanation: Using the lens formula 1/v - 1/u = 1/f, where u = -12 cm and f = -16 cm, we get v = -24 cm, indicating the beam diverges as if originating from 24 cm on the same side.
Explanation: Using the formula for critical angle, sin(θ_c) = n2/n1, where n1 = 1.5 and n2 = 1.33. Solving for θ_c gives sin⁻¹(1.33/1.5) ≈ 61.04°.
Explanation: Using the mirror equation, 1/f = 1/v + 1/u, where f = 15 cm and u = -12 cm. Solving for v gives v ≈ 6 cm (positive value indicates a virtual image behind the mirror).
Explanation: Magnification, m = -v/u = -6 cm / -12 cm = 0.5 (negative sign indicates the image is virtual and erect).
Explanation: Using Snell's Law, n1*sin(θ1) = n2*sin(θ2). Solving for θ2 gives sin⁻¹((1*sin(30°))/1.5) ≈ 19.47°.
Explanation: Using the formula for lens power, P = 1/f, where f is in meters. P = 1/0.5 = 2 diopters.
Explanation: Using the formula for apparent depth, n = real depth / apparent depth. Therefore, n = 12.5 cm / 9.4 cm ≈ 1.33.
Explanation: The magnifying power of a telescope is given by the ratio of the focal lengths of the objective and eyepiece. Therefore, magnifying power = 100 cm / 5 cm = 20.
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